.. _runs-mock: Uchuu Mock VLIM M★ — Run Summary ================================== Uchuu N-body mock catalogues are matched to the BGS VLIM M★ samples by density, redshift range, and stellar-mass threshold. The summary statistics are computed with ``measure_MOCK_VLIM_Mstar.ipynb``. **Cosmology:** Planck18 (H₀ = 67.4, Ω_m = 0.315) **Survey footprint:** 1/8 sky, RA ∈ [180°, 270°], Dec ∈ [−90°, 0°], area = **5 156.6 deg²**. **Redshift column:** ``redshift_S`` (spectroscopic-like). **Stellar mass column:** ``log₁₀(obs_sm)`` (SHAM-assigned masses). **Weights:** uniform (no systematic correction). .. note:: All samples use 100 jackknife regions (``N_JK=100``). Random catalogues are subsampled to 5 × N_gal before pair counting to keep corrfunc tree overhead manageable for small-volume samples. Sample inventory ---------------- .. list-table:: :header-rows: 1 :widths: 30 12 10 10 12 10 * - Sample key - N_gal - z_min - z_max - log₁₀M★_min - N_JK * - MOCK_VLIM_ANY_Mstar9.29_z0.05-0.08 - 155 846 - 0.05 - 0.08 - 9.29 - 100 * - MOCK_VLIM_ANY_Mstar9.78_z0.05-0.12 - 408 958 - 0.05 - 0.12 - 9.78 - 100 * - MOCK_VLIM_ANY_Mstar10.24_z0.05-0.18 - 781 950 - 0.05 - 0.18 - 10.24 - 100 * - MOCK_VLIM_ANY_Mstar10.45_z0.05-0.22 - 936 461 - 0.05 - 0.22 - 10.45 - 100 * - MOCK_VLIM_ANY_Mstar10.65_z0.05-0.26 - 923 373 - 0.05 - 0.26 - 10.65 - 100 * - MOCK_VLIM_ANY_Mstar10.84_z0.05-0.31 - 793 669 - 0.05 - 0.31 - 10.84 - 100 * - MOCK_VLIM_ANY_Mstar11.03_z0.05-0.35 - 460 808 - 0.05 - 0.35 - 11.03 - 100 * - MOCK_VLIM_ANY_Mstar11.22_z0.05-0.35 - 157 946 - 0.05 - 0.35 - 11.22 - 100 * - MOCK_VLIM_ANY_Mstar11.39_z0.05-0.35 - 50 067 - 0.05 - 0.35 - 11.39 - 100 Output files ------------ .. code-block:: text data/mocks/ ├── twopcf/{key}-wtheta.h5 w(θ) — Landy–Szalay, TreeCorr variance ├── twopcf/{key}-wp-pimax100.h5 wp(rp) — Landy–Szalay, TreeCorr variance ├── lf_smf/{key}-smf-vmax.h5 SMF — 1/Vmax, jackknife covariance └── joint/{key}-joint_smf_wp.h5 Joint SMF + wp, full jackknife covariance Sample characterisation ------------------------ Figures below are produced by ``make_mocks`` and show the match between the BGS observation (blue) and the Uchuu mock (orange). All 9 samples are now characterised. M★ ≥ 9.29 (N = 155 846, z < 0.08) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.29_Mstar_12.0_0.05_z_0.08_N_0155846_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥9.29 Sky footprint (RA/Dec) of the M★≥9.29 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.29_Mstar_12.0_0.05_z_0.08_N_0155846_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥9.29 Redshift (left) and stellar-mass (right) distributions for the M★≥9.29 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.29_Mstar_12.0_0.05_z_0.08_N_0155846_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥9.29 Stellar-mass vs. redshift plane for the M★≥9.29 mock and the corresponding BGS sample. M★ ≥ 9.78 (N = 408 958, z < 0.12) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.78_Mstar_12.0_0.05_z_0.12_N_0408958_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥9.78 Sky footprint (RA/Dec) of the M★≥9.78 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.78_Mstar_12.0_0.05_z_0.12_N_0408958_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥9.78 Redshift (left) and stellar-mass (right) distributions for the M★≥9.78 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_9.78_Mstar_12.0_0.05_z_0.12_N_0408958_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥9.78 Stellar-mass vs. redshift plane for the M★≥9.78 mock and the corresponding BGS sample. M★ ≥ 10.24 (N = 781 950, z < 0.18) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.24_Mstar_12.0_0.05_z_0.18_N_0781950_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥10.24 Sky footprint (RA/Dec) of the M★≥10.24 mock. The mock covers the southern Galactic octant (RA ∈ [180°, 270°], Dec < 0°). .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.24_Mstar_12.0_0.05_z_0.18_N_0781950_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥10.24 Redshift (left) and stellar-mass (right) distributions for the M★≥10.24 mock. Density is matched to within 0.001% of the observed value. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.24_Mstar_12.0_0.05_z_0.18_N_0781950_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥10.24 Stellar-mass vs. redshift plane for the M★≥10.24 mock and the corresponding BGS sample. M★ ≥ 10.45 (N = 936 461, z < 0.22) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.45_Mstar_12.0_0.05_z_0.22_N_0936461_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥10.45 Sky footprint (RA/Dec) of the M★≥10.45 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.45_Mstar_12.0_0.05_z_0.22_N_0936461_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥10.45 Redshift (left) and stellar-mass (right) distributions for the M★≥10.45 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.45_Mstar_12.0_0.05_z_0.22_N_0936461_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥10.45 Stellar-mass vs. redshift plane for the M★≥10.45 mock and the corresponding BGS sample. M★ ≥ 10.65 (N = 923 373, z < 0.26) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.65_Mstar_12.0_0.05_z_0.26_N_0923373_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥10.65 Sky footprint (RA/Dec) of the M★≥10.65 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.65_Mstar_12.0_0.05_z_0.26_N_0923373_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥10.65 Redshift (left) and stellar-mass (right) distributions for the M★≥10.65 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.65_Mstar_12.0_0.05_z_0.26_N_0923373_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥10.65 Stellar-mass vs. redshift plane for the M★≥10.65 mock and the corresponding BGS sample. M★ ≥ 10.84 (N = 793 669, z < 0.31) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.84_Mstar_12.0_0.05_z_0.31_N_0793669_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥10.84 Sky footprint (RA/Dec) of the M★≥10.84 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.84_Mstar_12.0_0.05_z_0.31_N_0793669_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥10.84 Redshift (left) and stellar-mass (right) distributions for the M★≥10.84 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_10.84_Mstar_12.0_0.05_z_0.31_N_0793669_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥10.84 Stellar-mass vs. redshift plane for the M★≥10.84 mock and the corresponding BGS sample. M★ ≥ 11.03 (N = 460 808, z < 0.35) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.03_Mstar_12.0_0.05_z_0.35_N_0460808_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥11.03 Sky footprint (RA/Dec) of the M★≥11.03 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.03_Mstar_12.0_0.05_z_0.35_N_0460808_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥11.03 Redshift (left) and stellar-mass (right) distributions for the M★≥11.03 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.03_Mstar_12.0_0.05_z_0.35_N_0460808_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥11.03 Stellar-mass vs. redshift plane for the M★≥11.03 mock and the corresponding BGS sample. M★ ≥ 11.22 (N = 157 946, z < 0.35) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.22_Mstar_12.0_0.05_z_0.35_N_0157946_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥11.22 Sky footprint (RA/Dec) of the M★≥11.22 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.22_Mstar_12.0_0.05_z_0.35_N_0157946_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥11.22 Redshift (left) and stellar-mass (right) distributions for the M★≥11.22 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.22_Mstar_12.0_0.05_z_0.35_N_0157946_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥11.22 Stellar-mass vs. redshift plane for the M★≥11.22 mock and the corresponding BGS sample. M★ ≥ 11.39 (N = 50 067, z < 0.35) ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.39_Mstar_12.0_0.05_z_0.35_N_0050067_compare_sky.png :width: 90% :alt: Sky footprint of mock M*≥11.39 Sky footprint (RA/Dec) of the M★≥11.39 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.39_Mstar_12.0_0.05_z_0.35_N_0050067_compare_1D.png :width: 90% :alt: Redshift and mass distributions M*≥11.39 Redshift (left) and stellar-mass (right) distributions for the M★≥11.39 mock. .. figure:: ../figures/runs/MOCK_VLIM_ANY_11.39_Mstar_12.0_0.05_z_0.35_N_0050067_compare_zMstar.png :width: 90% :alt: z-M* plane M*≥11.39 Stellar-mass vs. redshift plane for the M★≥11.39 mock and the corresponding BGS sample. Stellar mass function --------------------- .. figure:: ../figures/runs/mock_smf_overlay.png :width: 90% :alt: Mock SMF overlay Stellar mass function φ(M★) for all 9 Uchuu mock VLIM samples, estimated with the 1/Vmax method (coloured markers with jackknife errors). The cosmological area (5 156.6 deg²) is used for normalisation. Literature references overlaid as dashed/dotted lines: Baldry+2012 GAMA I, Driver+2022 GAMA DR4, Moustakas+2013 PRIMUS z<0.2, Xu+2025 DESI PAC (shaded band). See :ref:`literature` for provenance. SMF key values at the lowest complete stellar mass bin: .. list-table:: :header-rows: 1 :widths: 30 10 12 22 22 * - Sample - log₁₀M★_min - z_max - log₁₀M★_ref [dex] - φ [Mpc⁻³ dex⁻¹] * - MOCK_VLIM_ANY_Mstar9.29 - 9.29 - 0.08 - 9.38 - 7.00 × 10⁻³ ± 1.6 × 10⁻⁴ * - MOCK_VLIM_ANY_Mstar9.78 - 9.78 - 0.12 - 9.88 - 5.53 × 10⁻³ ± 9.2 × 10⁻⁵ * - MOCK_VLIM_ANY_Mstar10.24 - 10.24 - 0.18 - 10.12 - 1.92 × 10⁻⁴ ± 2.9 × 10⁻⁶ * - MOCK_VLIM_ANY_Mstar10.45 - 10.45 - 0.22 - 10.38 - 8.67 × 10⁻⁴ ± 1.1 × 10⁻⁵ * - MOCK_VLIM_ANY_Mstar10.65 - 10.65 - 0.26 - 10.62 - 1.56 × 10⁻³ ± 1.6 × 10⁻⁵ * - MOCK_VLIM_ANY_Mstar10.84 - 10.84 - 0.31 - 10.88 - 1.51 × 10⁻³ ± 1.3 × 10⁻⁵ * - MOCK_VLIM_ANY_Mstar11.03 - 11.03 - 0.35 - 11.12 - 8.84 × 10⁻⁴ ± 9.2 × 10⁻⁶ * - MOCK_VLIM_ANY_Mstar11.22 - 11.22 - 0.35 - 11.12 - 7.88 × 10⁻⁵ ± 8.9 × 10⁻⁷ * - MOCK_VLIM_ANY_Mstar11.39 - 11.39 - 0.35 - 11.38 - 7.38 × 10⁻⁵ ± 9.2 × 10⁻⁷ Angular correlation function w(θ) ---------------------------------- .. figure:: ../figures/runs/mock_wtheta_overlay.png :width: 90% :alt: Mock w(theta) overlay Angular two-point correlation function w(θ) for all 9 mock samples, measured with the Landy–Szalay estimator. Error bars are TreeCorr variance estimates. Bins: 30 log-spaced bins in [0.01, 60] arcmin. Projected correlation function w\ :sub:`p`\ (r\ :sub:`p`) ----------------------------------------------------------- .. figure:: ../figures/runs/mock_wp_overlay.png :width: 90% :alt: Mock wp overlay Projected correlation function w\ :sub:`p`\ (r\ :sub:`p`) for all 9 mock samples (π\ :sub:`max` = 100 Mpc), measured with Corrfunc Landy–Szalay. Error bars are jackknife uncertainties from the joint covariance. Bins: 30 log-spaced bins in [0.01, 60] Mpc. Representative w\ :sub:`p`\ (r\ :sub:`p`) values at r\ :sub:`p` = 1 Mpc and 10 Mpc (from the joint covariance files, uniform weights): .. list-table:: :header-rows: 1 :widths: 35 10 22 22 * - Sample - log₁₀M★_min - w\ :sub:`p`\ (1 Mpc) [Mpc] - w\ :sub:`p`\ (10 Mpc) [Mpc] * - MOCK_VLIM_ANY_Mstar9.29 - 9.29 - 164.8 ± 20.5 - 19.0 ± 14.1 * - MOCK_VLIM_ANY_Mstar9.78 - 9.78 - 201.4 ± 15.7 - 26.4 ± 11.8 * - MOCK_VLIM_ANY_Mstar10.24 - 10.24 - 222.6 ± 10.5 - 29.6 ± 7.8 * - MOCK_VLIM_ANY_Mstar10.45 - 10.45 - 238.6 ± 8.4 - 32.9 ± 7.3 * - MOCK_VLIM_ANY_Mstar10.65 - 10.65 - 255.1 ± 7.2 - 34.5 ± 5.2 * - MOCK_VLIM_ANY_Mstar10.84 - 10.84 - 274.8 ± 8.3 - 36.5 ± 6.7 * - MOCK_VLIM_ANY_Mstar11.03 - 11.03 - 317.4 ± 6.8 - 40.7 ± 3.9 * - MOCK_VLIM_ANY_Mstar11.22 - 11.22 - 395.7 ± 11.8 - 49.5 ± 4.4 * - MOCK_VLIM_ANY_Mstar11.39 - 11.39 - 571.4 ± 40.7 - 65.1 ± 6.6 Joint SMF + w\ :sub:`p` covariance ------------------------------------ The joint covariance matrix is estimated with 100-region spatial jackknife resampling. The data vector is :math:`\mathbf{d} = [\phi_1,\ldots,\phi_{N_\mathrm{SMF}},\, w_p^1,\ldots,w_p^{N_{w_p}}]`. .. figure:: ../figures/runs/mock_joint_corrmat.png :width: 100% :alt: Mock joint correlation matrices Pearson correlation matrices of the joint SMF + w\ :sub:`p` data vector for all 9 mock samples. The dashed line separates the SMF (top-left) from the w\ :sub:`p` (bottom-right) blocks. Off-diagonal cross-correlations encode the covariance between the two statistics. Regenerating figures --------------------- After new results are available, re-run:: python docs/scripts/make_run_figures.py cd docs && make html